000			03019nam a22005415i 4500
001			978-3-540-46971-1
003			DE-He213
005			20160624101851.0
007			cr nn 008mamaa
008			121227s1990 gw | s |||| 0|eng d
020			_a9783540469711 _9978-3-540-46971-1
024	7		_a10.1007/BFb0036058 _2doi
050		4	_aQB4
072		7	_aPG _2bicssc
072		7	_aSCI004000 _2bisacsh
072		7	_aNAT033000 _2bisacsh
082	0	4	_a520 _223
245	1	0	_aAccuracy of Element Abundances from Stellar Atmospheres _h[electronic resource] : _bProceedings of Two Sessions Allocated at the IAU General Assembly in Baltimore, USA, August 1988 / _cedited by Rainer Wehrse.
260		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1990.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1990.
300			_aV, 109 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aLecture Notes in Physics, _x0075-8450 ; _v356
505	0		_aOn the accuracy of atomic transition probabilities -- Accuracy of excitation and ionisation cross sections -- Accuracy of line broadening data -- Accuracy of abundances from O to mid B main sequence stars -- The accuracy of abundances from middle B to F main sequence normal stars -- Accuracy of the determination of the abundances in solar type stars -- Problems associated with cool dwarf stars -- Accuracy of abundances from stars in near-by galaxies.
520			_aTo get a reasonably realistic picture of the structure and evolution of stars one needs to know accurately the abundances of chemical elements and their isotopes in the stellar atmosphere and in the galactic environment of the stars. The articles collected in this volume give a modern review of the abundance accuracies for main-sequence stars. After a general introduction in the first part the accuracies of atomic transition probabilities, ionization and excitation cross-sections, and line broad- ening data are discussed. In the second part the specific problems and results for different stellar types are presented, and, finally, an overview on the possibilities of abundance determinations for stars outside the Galaxy is given.
650		0	_aPhysics.
650		0	_aPhysical geography.
650		0	_aAstronomy.
650		0	_aAstrophysics.
650		0	_aSpectrum analysis.
650	1	4	_aPhysics.
650	2	4	_aAstronomy.
650	2	4	_aAstrophysics.
650	2	4	_aOptical Spectroscopy, Ultrafast Optics.
650	2	4	_aGeophysics/Geodesy.
700	1		_aWehrse, Rainer. _eeditor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9783540523659
786			_dSpringer
830		0	_aLecture Notes in Physics, _x0075-8450 ; _v356
856	4	0	_uhttp://dx.doi.org/10.1007/BFb0036058
942			_2EBK2591 _cEBK
999			_c31885 _d31885